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Practical_Antenna_Handbook_0071639586

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I n d e x 757<br />

noise (Cont.):<br />

sky noise, 494–495, 498<br />

solar, 49<br />

noise bridge, 592–598<br />

noise factor (F n ), 492–493<br />

noise figure (NF), 492–494<br />

noise temperature (T e ), 493–495<br />

nonresonant longwire, 256–258<br />

nonresonant loop, 365–366<br />

nonresonant rhombic, 260, 262<br />

nonresonant vee beam, 260, 261<br />

normalized impedance, 559–562, 574<br />

northern lights, 75–76<br />

nulls (loop antenna), 342–346, 359<br />

Numerical Electromagnetic Computation<br />

(NEC) program, 546<br />

O<br />

off-Âcenter-Âfed dipole, 225–226<br />

ohm (Ω unit of resistance), 82–83<br />

ohmic loss, 28, 107, 178, 447, 449, 473<br />

ohmmeter (coaxial cable test), 615–616<br />

Ohm’s law, 82–83, 686<br />

in transmission lines, 125<br />

omega (Ω), 115, 715<br />

omega-Âmatch feed systems, 244–246<br />

omnidirectional, 265–266<br />

1λ loops, 209–216<br />

open-Âwire line (OWL), 110–111, 687, 689<br />

ordinances, 701<br />

Orr, William, Âex-ÂW6SAI, 277<br />

OSCAR satellite communications, 6<br />

oscilloscope, 127–131, 712<br />

(See also transmission lines)<br />

P<br />

parabolic (dish) antennas, 481–485<br />

beamwidth, 483<br />

Cassegrain feed, 483–484<br />

directrix, 481–482<br />

effective aperture, 483<br />

feed geometries for, 483–485<br />

gain, 483<br />

monopulse feed, 483, 485<br />

parallel conductor lines 110–111<br />

(See also Âopen-Âwire line)<br />

parasitic arrays, 161–162, 277, 280–282, 419<br />

path loss, 18<br />

pedestal (tower), 669–671<br />

pennant antenna, 359–360<br />

period (T; of a waveform), 712, 715<br />

permeability (µ), 90, 116, 460<br />

relative (µ r ), 90<br />

permittivity (ε; dielectric constant), 88, 105,<br />

116–118, 460<br />

relative (ε r ), 88<br />

phase, 91, 100, 150<br />

phase constant (β), 120, 140–142<br />

phase-Âcontrol circuit, 340–341<br />

phase-Âlocked receivers, 68<br />

phase-Âshift networks, 156, 267–271, 485–487<br />

phase velocity (V p ), 455–458<br />

phasing, 149–153, 158–159, 266, 273, 340–341<br />

physical vs. electrical length, 105, 140, 176–177<br />

pi network, 537<br />

“picket fencing,” 32<br />

planar loop windings, 345<br />

planetary terminator (See gray line<br />

propagation)<br />

planning board, 702–703<br />

“plumbers’ delight” Yagi, 277<br />

polarity, 82, 88, 99, 104<br />

polarization, 18–19, 229, 473<br />

polarization diversity, 67–68, 331–332<br />

Popov, Alexander, 3<br />

pop rivets, 290, 296<br />

power (P), 83<br />

(See also effective radiated power)<br />

power density, 16–17, 471–472<br />

power distribution, 683, 689–690<br />

power gain (G p ), 477–478, 710–711<br />

preamplifier for receiving antennas, 355–356<br />

PRB-1 (FCC), 700<br />

predictions, propagation, 76–79<br />

propagation constant (β), 462<br />

propagation modes in waveguides, 451–454<br />

propagation of radio waves, 9–79<br />

ducting, 39–40, 42<br />

fading, 41–42<br />

ground wave, 27–38<br />

ionospheric (see ionospheric propagation)<br />

inversion, 39<br />

line of sight, 28<br />

medium, 12–13<br />

meteor scatter, 76<br />

path types, 26–27<br />

radio horizon, 32, 39<br />

subrefraction, 40

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